HP2 survey: III The California Molecular Cloud--A Sleeping Giant Revisited

Author(s)

Charles J. Lada, John A. Lewis, Marco Lombardi, João Alves

Abstract

We present new high resolution and dynamic range dust column density and temperature maps of the California Molecular Cloud derived from a combination of Planck and Herschel dust-emission maps, and 2MASS NIR dust-extinction maps. We used these data to determine the ratio of the 2.2 μm extinction coefficient to the 850 μm opacity and found the value to be close to that found in similar studies of the Orion B and Perseus clouds but higher than that characterizing the Orion A cloud, indicating that variations in the fundamental optical properties of dust may exist between local clouds. We show that over a wide range of extinction, the column density probability distribution function (pdf) of the cloud can be well described by a simple power law (i.e., PDF N A K -n) with an index (n = 4.0 ± 0.1) that represents a steeper decline with A K than found (n 3) in similar studies of the Orion and Perseus clouds. Using only the protostellar population of the cloud and our extinction maps we investigate the Schmidt relation, that is, the relation between the protostellar surface density, Σ -, and extinction, A K, within the cloud. We show that Σ - is directly proportional to the ratio of the protostellar and cloud pdfs, i.e., PDF -(A K)/PDF N(A K). We use the cumulative distribution of protostars to infer the functional forms for both Σ - and PDF -. We find that Σ - is best described by two power-law functions. At extinctions A K2.5 mag, Σ -A K β with β = 3.3 while at higher extinctions β = 2.5, both values steeper than those (2) found in other local giant molecular clouds (GMCs). We find that PDF - is a declining function of extinction also best described by two power-laws whose behavior mirrors that of Σ -. Our observations suggest that variations both in the slope of the Schmidt relation and in the sizes of the protostellar populations between GMCs are largely driven by variations in the slope, n, of PDF N(A K). This confirms earlier studies suggesting that cloud structure plays a major role in setting the global star formation rates in GMCs.

Organisation(s)

Department of Astrophysics

External organisation(s)

Harvard-Smithsonian Center for Astrophysics, Università degli Studi di Milano-Bicocca

Journal

Astronomy & Astrophysics

Volume

606

No. of pages

16

ISSN

0004-6361

DOI

https://doi.org/10.1051/0004-6361/201731221

Publication date

10-2017

Peer reviewed

Yes

Austrian Fields of Science 2012

103004 Astrophysics

Keywords

ASJC Scopus subject areas

Astronomy and Astrophysics, Space and Planetary Science

Portal url

https://ucrisportal.univie.ac.at/en/publications/1e7b2df0-ff6b-4ebd-b5cf-2f6a3bdc4db1